Computer Science – Performance
Scientific paper
Jun 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..405..539k&link_type=abstract
Solar Polarization 5: In Honor of Jan Stenflo ASP Conference Series, Vol. 405, proceedings of the conference held 17-21 Septembe
Computer Science
Performance
1
Scientific paper
We present a new implementation of the magnetic Doppler imaging technique, which aims at self-consistent temperature and magnetic mapping of the surface structures in cool active stars. Our magnetic imaging procedure is unique in its capability to model individual spectral features in all four Stokes parameters. We discuss performance and intrinsic limitations of the new magnetic Doppler imaging method. A special emphasis is given to the simultaneous modeling of the magnetically sensitive lines in the optical and infrared regions and to combining information from both atomic and molecular spectral features. These two techniques may, for the first time, give us a tool to study magnetic fields in the starspot interiors.
Kochukhov Oleg
Piskunov Nicolai
No associations
LandOfFree
Magnetic Doppler Imaging of Active Stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Magnetic Doppler Imaging of Active Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetic Doppler Imaging of Active Stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1068521